%ForeignArg-I-=, ======== %ForeignArg-I-Arg 1, smei=/home/soft/dat/smei/low_res/*.* %ForeignArg-I-Arg 2, nagoya=nagoya,,yearly %ForeignArg-I-Arg 3, ace=/home/soft/dat/insitu/acesw_[4].hravg %ForeignArg-I-Arg 4, nso_sorr=/home/soft/dat/map/nso_noaa/hcss/nso_noaa[4]_[3].f ts %ForeignArg-I-=, ======== %MAP_TZERO-I-JDCar, Start yr 1974, doy 333.073 (JD 2442380.6) %MAP_TZERO-I-JDCar, End yr 2027, doy 40.609 (JD 2461446.1) The max CR # and lower and upper JD 700 2442380.57336426 2461446.10937500 NCoff = 1621 Forecast mode? (YES/NO) < NO > Number of iterations? < 18 > Deconvolution distance (AU; 0=solar surface)? < -15 > Deconvolve: velocity, density, both < both > Use velocity data from: Nagoya, Ooty < Nagoya > Minimum number of velocity lines of sight? < 200 > Use in-situ velocity data in 3D reconstructions? (YES/NO) < YES > Use in-situ velocity data from: ACE_L0, ACE_L2, Wind, CELIAS < ACE_L0 > Minimum velocity for in-situ velocity values < 100 > Maximum velocity for in-situ velocity values < 1500 > Use density or G-level data from: SMEI, Nagoya, Ooty < SMEI >%MAP_TZERO-I-JDCar, Start yr 1974, doy 333.07 (JD 2442380.6) %MAP_TZERO-I-JDCar, End yr 2027, doy 40.609 (JD 2461446.1) Use in-situ density data in the 3D reconstructions? (YES/NO) < YES > Use in-situ density data from: ACE_L0, ACE_L2, Wind, CELIAS < ACE_L0 > Fit in-situ density data to ACE level 0 data (YES/NO) < YES > Minimum density for fit in-situ density values < 1E-2 > Maximum density for fit in-situ density values < 100 > Fit average in-situ density data to brigntness? (YES/NO) < YES > Use in-situ density in tomography (YES/NO) < YES > The directory used for the SMEI tomography analysis follows: /home/soft/dat/smei/low_res/*.* /home/soft/dat/insitu/acesw_????.hravg Deconvolve V from one day to the next? (YES/NO) < YES > Number of days to combine for velocity? < 0.5 > Number of hours from V UT midnight? < -9 > Number of velocity time values? < 109 > Deconvolve V from one day to the next (YES/NO) < YES > Number of days to combine for velocity? < 0.5 > Number of hours from V UT midnight? < -9 > Number of velocity time values? < 109 > Deconvolve density or G from one day to the next (YES/NO) < YES > Number of days to combine for density or G-level? < 0.5 > Number of hours from density or G UT midnight? < 0 > Number of density or G-level time values? < 109 > Iteration at which to limit V-source deviations, -1=none < 9 > All velocity data, East data, West data ? < All velocity data > Please, select from range [0,180] Minimum elongation for V-data < 11.5 > Please, select from range [11.5,180] Maximum elongation for V-data < 180 > Please, select from range [600,1000] Anti-Earth maximum velocity at 1 AU < 800 > Please, select from range [0,400] Anti-Earth minimum velocity at 1 AU < 200 > Please, select from range [90,180] Angular distance from Earth to begin V limit < 135 > Please, select from range [0,180] Maximum RA relative to Sun for V-data < 90 > V-map reference distance in AU (0=solar surface)? < 6.97861004E-2 > Do you want to use a proxy map for velocity? (YES/NO) < NO > Maximum upper limit for tomography velocity? < 1200 > Maximum lower limit for tomography velocity? < 100 > Maximum upper limit for source velocity? < 1200 > Maximum lower limit for source velocity? < 100 > Iteration at which to limit D or G-source deviations, -1=none < 9 > All D or G data, East data, West data ? < All D or G data > Please, select from range [0,180] Minimum elongation for D or G-data < 15 > Please, select from range [15,180] Maximum elongation for D or G-data < 180 > Please, select from range [5,30] Anti-Earth maximum density at 1 AU < 10 > Please, select from range [0,4] Anti-Earth minimum density at 1 AU < 2 > Please, select from range [90,180] Angular distance from Earth to begin D limit < 90 > Please, select from range [0,180] Maximum RA relative to Sun for D or G-data < 180 > D or G-map reference distance in AU (0=solar surface)? < 6.97861004E-2 > Do you want to use a proxy map for density? (YES/NO) < NO > Maximum limit for D or G deconvolution? < 5 > Minimum limit for D or G deconvolution? < -2 > Factor by which to modify brightness? < 1 > Density spatial filter (degrees)? < 4.66666985 > Density temporal filter (days)? < 0.375 > Density time hole filter? < 1 > # of D or G-points per bin that constitute a deconvolution < 1.5 > Velocity spatial filter (degrees)? < 14 > Velocity temporal filter (days)? < 0.75 > Velocity time hole filter? < 1 > # of V-points per bin that constitute a deconvolution < 0.175 > 1 AU average density to fit base? < 5 > G-level power to fit velocity? < 0.34999999 > Radial Density falloff? < 2 > Radial G-level falloff to fit V density? < 0.30000001 > Solar wind speed for G-level traceback? < 400 > Carrington rotation (0 = STOP)90 < 2003 > # Rotations averaged < 1 > Carrington rotation 2003 starts on date 13-MAY-2003 ( Doy 133 ) %MAP_TZERO-I-JDCar, Start yr 2003, doy 23.943 (JD 2452663.4) %MAP_TZERO-I-JDCar, End yr 2055, doy 96.461 (JD 2471729) Beginning SMEI orbit # = 1744 Number of orbits = 695 Do you want to output model-source files (YES/NO) < NO > Do you want to output l.o.s. source surface maps (YES/NO) < NO > Do you want one shift matrix per iteration (YES/NO) < NO > Output good source files (YES/NO) < NO > Output three D error files (YES/NO) < YES > Output a three D file (YES/NO) < NO > Output a three D high resolution file (YES/NO) < YES > How many intervals do you want to specify (up to 3)? < 0 > Minimum high-resolution height in AU? < 6.97861004E-2 > Maximum high-resolution height in AU? < 1.5 > Do you want the density error to limit HR densities? (YES/NO) < YES > What density L.O.S. crossing limit? < 10 > Do you want the density error to limit HR velocities (YES/NO) < YES > Do you want the velocity error to limit HR velocities (YES/NO) < NO > Output completely filled three D files (YES/NO) < NO > Output a Three D high resolution base (YES/NO) < YES > How many intervals do you want to specify (up to 3)? < 0 > Minimum high-resolution base height in AU? < 6.97861004E-2 > Maximum high-resolution base height in AU? < 1.5 > Do you want the density error to limit HR densities (YES/NO) < YES > What density L.O.S. crossing limit? < 10 > Do you want the density error to limit HR velocities (YES/NO) < YES > Do you want the velocity error to limit HR velocities (YES/NO) < NO >%BField_Choose_3-I-nso_sorr, maps in /home/soft/dat/map/nso_noaa/hcss/nso_noaa?? ??_???.fts Do you want to make magnetic source surface maps? (YES/NO) < YES > True bWildMag(J) J = 9 T Do you want to produce magnetic field 3D files? (YES/NO) < YES > Do you want to extract magnetic fields? (YES/NO) < NO > Multiplicative factor for CSSS fields? < 2 > Adjust field factors for possible known effects? (YES/NO) < NO > Output an Earth parameter file (YES/NO) < YES > Output a Mercury parameter file (YES/NO) < NO >